Small, Young Fluvial Features in Icy Terrains on Mars

Details Small, Young Fluvial Features in Icy Terrains on Mars Small, Young Fluvial Features in Icy Terrains on Mars

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1185f&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

We describe small valleys found in association with ice-rich terrains on
Mars (lobate debris aprons and viscous flow features). The most probable
mechanism for their formation is the melting of ice, likely during the
Amazonian.

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